Radio Weak Lensing Shear Measurement in the Visibility Domain - I. Methodology

TL;DR

This paper introduces a radio-specific adaptation of the lensfit shear measurement method, working directly in the visibility domain to improve weak lensing analysis with upcoming radio telescopes like SKA.

Contribution

It develops a Bayesian likelihood approach for galaxy shape measurement directly from radio interferometer visibilities, avoiding imaging systematics and demonstrating feasibility with simulated SKA data.

Findings

Bias estimates are within SKA1 requirements for high SNR.

Shear measurement biases are comparable to optical surveys at moderate SNR.

Method shows promise for future radio weak lensing surveys.

Abstract

The high sensitivity of the new generation of radio telescopes such as the Square Kilometre Array (SKA) will allow cosmological weak lensing measurements at radio wavelengths that are competitive with optical surveys. We present an adaptation to radio data of lensfit, a method for galaxy shape measurement originally developed and used for optical weak lensing surveys. This likelihood method uses an analytical galaxy model and makes a Bayesian marginalisation of the likelihood over uninteresting parameters. It has the feature of working directly in the visibility domain, which is the natural approach to adopt with radio interferometer data, avoiding systematics introduced by the imaging process. As a proof of concept, we provide results for visibility simulations of individual galaxies with flux density S >= 10 muJy at the phase centre of the proposed SKA1-MID baseline configuration, adopting 12 frequency channels in the band 950 - 1190 MHz. Weak lensing shear measurements from a population of galaxies with realistic flux and scalelength distributions are obtained after natural gridding of the raw visibilities. Shear measurements are expected to be affected by "noise bias": we estimate the bias in the method as a function of signal-to-noise ratio (SNR). We obtain additive and multiplicative bias values that are comparable to SKA1 requirements for SNR > 18 and SNR > 30, respectively. The multiplicative bias for SNR > 10 is comparable to that found in ground-based optical surveys such as CFHTLenS, and we anticipate that similar shear measurement calibration strategies to those used for optical surveys may be used to good effect in the analysis of SKA radio interferometer data.